- Solar Phys (2007) 240: 3748 DOI 10.1007/s11207-006-0247-6
- Solar Physics (2006) 235: 201221 DOI: 10.1007/s11207-006-0065-x C Springer 2006
- MAGNETIC MODELING AND TOMOGRAPHY: FIRST STEPS TOWARDS A CONSISTENT RECONSTRUCTION OF THE SOLAR
- A&A 453, 737741 (2006) DOI: 10.1051/0004-6361:20054751
- Solar Phys (2008) 248: 379393 DOI 10.1007/s11207-007-9027-1
- A&A 484, 495502 (2008) DOI: 10.1051/0004-6361:200809508
- Solar Physics (2006) 236: 2540 DOI: 10.1007/s11207-006-0153-y C Springer 2006
- A&A 503, 991997 (2009) DOI: 10.1051/0004-6361/200912066
- A&A 481, 827834 (2008) DOI: 10.1051/0004-6361:20078834
- The Astrophysical Journal Letters, 716:L68L73, 2010 June 10 doi:10.1088/2041-8205/716/1/L68 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- Magnetic Stereoscopy of Coronal loops in NOAA 8891 L. Feng1,2, T. Wiegelmann1, B. Inhester1, S. Solanki1, W.Q. Gan2, P.
- Solar Phys (2007) 240: 227239 DOI 10.1007/s11207-006-0266-3
- Solar Physics (2005) 228: 6778 C Springer 2005 HOW TO USE MAGNETIC FIELD INFORMATION FOR CORONAL
- OPTIMIZATION CODE WITH WEIGHTING FUNCTION FOR THE RECONSTRUCTION OF CORONAL MAGNETIC FIELDS
- Nonlinear force-free modeling of the solar coronal magnetic field
- HELMET STREAMERS WITH TRIPLE STRUCTURES: WEAKLY TWO-DIMENSIONAL STATIONARY STATES
- INCLUDING STEREOSCOPIC INFORMATION IN THE RECONSTRUCTION OF CORONAL MAGNETIC FIELDS
- A&A 428, 629645 (2004) DOI: 10.1051/0004-6361:20041060
- Solar Physics (2004) 225: 227247 C Springer 2005 SIMILARITIES AND DIFFERENCES BETWEEN CORONAL HOLES
- A&A 433, 701705 (2005) DOI: 10.1051/0004-6361:20042421
- A&A 432, L1L4 (2005) DOI: 10.1051/0004-6361:200500029
- Solar Physics (2006) 233: 215232 DOI: 10.1007/s11207-006-2092-z C Springer 2006
- A&A 457, 10531058 (2006) DOI: 10.1051/0004-6361:20065281
- A&A 475, 701706 (2007) DOI: 10.1051/0004-6361:20078244
- A&A 488, L71L74 (2008) DOI: 10.1051/0004-6361:200810235
- PLASMA FLOWS GUIDED BY STRONG MAGNETIC FIELDS IN THE SOLAR CORONA Eckart Marsch
- STUDY OF MAGNETIC CHANNEL STRUCTURE IN ACTIVE REGION 10930 Haimin Wang,1, 2
- Multiple-spacecraft study of an extended magnetic structure in the solar wind
- The Astrophysical Journal, 696:8490, 2009 May 1 doi:10.1088/0004-637X/696/1/84 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- The Astrophysical Journal, 696:15261532, 2009 May 10 doi:10.1088/0004-637X/696/2/1526 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- The Astrophysical Journal, 700:292301, 2009 July 20 doi:10.1088/0004-637X/700/1/292 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- Ann. Geophys., 27, 29252936, 2009 www.ann-geophys.net/27/2925/2009/
- A&A 508, 421432 (2009) DOI: 10.1051/0004-6361/200912529
- A&A 511, A4 (2010) DOI: 10.1051/0004-6361/200912812
- The Astrophysical Journal, 713:440449, 2010 April 10 doi:10.1088/0004-637X/713/1/440 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- The Astrophysical Journal, 714:343354, 2010 May 1 doi:10.1088/0004-637X/714/1/343 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
- Astronomy & Astrophysics manuscript no. aa14391-10 c ESO 2010 May 10, 2010
- Solar Phys (2008) 247: 269299 DOI 10.1007/s11207-007-9110-7
- HELMET STREAMERS WITH TRIPLE STRUCTURES: SIMULATIONS OF RESISTIVE DYNAMICS
- The Astrophysical Journal, 671: L205L208, 2007 December 20 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
- Source region of the 18 November 2003 coronal mass ejection that led to the strongest magnetic storm of cycle 23
- A QUANTITATIVE METHOD TO OPTIMISE MAGNETIC FIELD LINE FITTING OF OBSERVED CORONAL LOOPS
